Fiscal Year 2002 Performance and Accountability Report
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Deep Space Craft an Overview of Interplanetary Flight Dave Doody Deep Space Craft an Overview of Interplanetary Flight
Deep Space Craft An Overview of Interplanetary Flight Dave Doody Deep Space Craft An Overview of Interplanetary Flight Published in association with PPraxisraxis PPublishiublishingng Chichester, UK Dave Doody NASA Jet Propulsion Laboratory (Caltech) Pasadena California USA Front cover illustrations: (Upper) Artist's rendition of the Dawn spacecraft operating its ion propulsion system upon arrival at the main-belt asteroid Vesta in 2011. Image courtesy McRel, Mid-continent Research for Education and Learning. (Next lower) Artist's concept of the Phoenix lander operating in the Martian Arctic, as it did from May to November 2008. Image courtesy University of Arizona. (Lower left) Artist's concept of the Cassini spacecraft as it operates in Saturn orbit July 2004 through the present day. Back cover illustrations: (Left) A near-duplicate of the Mars Phoenix lander used in developing command sequences before being sent to the spacecraft. Here, members of the Robotic Arm Engineering Team test the arm's motorized raft in the Payload Interoperability Testbed at the University of Arizona, Tucson in July 2008. Image courtesy University of Arizona. (Right) Rob Manning, Chief Engineer of NASA's Mars Exploration Program, cheers along with other team members as the ®rst images from rover Spirit come back from Mars. Courtesy NASA/Bill Ingalls. SPRINGER±PRAXIS BOOKS IN ASTRONAUTICAL ENGINEERING SUBJECT ADVISORY EDITOR: John Mason M.B.E., B.Sc., M.Sc., Ph.D. ISBN 978-3-540-89509-1 Springer Berlin Heidelberg New York Springer is part of Springer-Science + Business Media (springer.com) Library of Congress Control Number: 2008943657 Apart from any fair dealing for the purposes of research or private study, or criticism or review, as permitted under the Copyright, Designs and Patents Act 1988, this publication may only be reproduced, stored or transmitted, in any form or by any means, with the prior permission in writing of the publishers, or in the case of reprographic reproduction in accordance with the terms of licences issued by the Copyright Licensing Agency. -
Image – Action – Space
Image – Action – Space IMAGE – ACTION – SPACE SITUATING THE SCREEN IN VISUAL PRACTICE Luisa Feiersinger, Kathrin Friedrich, Moritz Queisner (Eds.) This publication was made possible by the Image Knowledge Gestaltung. An Interdisciplinary Laboratory Cluster of Excellence at the Humboldt-Universität zu Berlin (EXC 1027/1) with financial support from the German Research Foundation as part of the Excellence Initiative. The editors like to thank Sarah Scheidmantel, Paul Schulmeister, Lisa Weber as well as Jacob Watson, Roisin Cronin and Stefan Ernsting (Translabor GbR) for their help in editing and proofreading the texts. This work is licensed under a Creative Commons Attribution-NonCommercial-No-Derivatives 4.0 License. For details go to https://creativecommons.org/licenses/by-nc-nd/4.0/. Copyrights for figures have been acknowledged according to best knowledge and ability. In case of legal claims please contact the editors. ISBN 978-3-11-046366-8 e-ISBN (PDF) 978-3-11-046497-9 e-ISBN (EPUB) 978-3-11-046377-4 Library of Congress Control Number: 2018956404 Bibliographic information published by the Deutsche Nationalbibliothek The Deutsche National bibliothek lists this publication in the Deutsche Nationalbibliographie; detailed bibliographic data are available on the internet at http://dnb.dnb.de. © 2018 Luisa Feiersinger, Kathrin Friedrich, Moritz Queisner, published by Walter de Gruyter GmbH, Berlin/Boston The book is published with open access at www.degruyter.com, https://www.doabooks.org and https://www.oapen.org. Cover illustration: Malte Euler Typesetting and design: Andreas Eberlein, aromaBerlin Printing and binding: Beltz Bad Langensalza GmbH, Bad Langensalza Printed in Germany www.degruyter.com Inhalt 7 Editorial 115 Nina Franz and Moritz Queisner Image – Action – Space. -
Mp-Avt-171-09
UNCLASSIFIED/UNLIMITED Attitude Determination and Control of Future Small Satellites H. Ersin Soken, A. Rustem Aslan and Chingiz Hajiyev Aeronautics and Astronautics Faculty Istanbul Technical University Istanbul, TURKEY [email protected]/[email protected]/[email protected] ABSTRACT As well as other subsystems, Attitude Determination and Control System (ADCS) development is a challenging process for small satellites because of design limitations, such as size, weight and the power consumption. Besides, if they are thought in a concept with military missions, then the requirement for a high attitude pointing accuracy is something certain. Works on the effective attitude determination and control methods for small satellites can be accepted as a part of this struggle. In this paper, problems that are met during ADCS development phase for future small satellites are stated and possible solutions are suggested. 1.0 INTRODUCTION Since their first appearance, small satellites have begun to play a more and more important role in space researches and today, they have a certain share in astronautic applications, especially about new technology demonstration. Because of many advantages such as low investment and operational costs, enabling COTS (commercial of the shell) technology in space, short system development periods etc. they have been highly preferred to their larger competitors. More than 400 micro satellites launched in the last 20 years is a good proof for that [1]. Mini Satellite 100-500 kg Micro Satellite 10-100 kg Nano Satellite 1-10 kg Pico Satellite 0.1-1 kg Table 1: Small satellite classification. Although they have been investigated in depth, there are still many steps to be taken in the development phase of these types of satellites and an important field to be examined is their attitude determination and control systems (ADCS). -
JPL Has Once Again Closed out the Year in Style. Less Than a Month
Jet DECEMBER Propulsion 2006 Laboratory VOLUME 36 NUMBER 17 2006 INREVIEW By Mark Whalen JPL has once again closed out the year in style. Less than a month after the announcement that Mars Global Surveyor has likely finished its operat- ing career, the most productive Mars mission in history came through with the explosive news in December that its photographs have revealed bright new deposits in two gullies on Mars that suggest water carried sediment A gully as imaged by Mars Global Surveyor liquid water was involved in its genesis. through them sometime during the is shown at left in August 1999 and at right However, this observation and a similar in September 2005. The images show the light-toned flow in Terra Sirenum to- past seven years. southeast wall of an unnamed crater in the gether show that some gully sites are Centauri Montes region. No light-toned indeed changing today, providing tanta- In the meantime, the Laboratory con- deposit was present in August 1999, but lizing evidence there might be sources of appeared by February 2004. The new light- liquid water beneath the surface of Mars tinues its studies of the solar system toned flow, by itself, does not prove that right now. and beyond, with 15 spacecraft, two rovers, seven science instruments and three Earth observatories all meeting or exceeding their require- ments. Following are some highlights, chronologically, from 2006. Continued on page 2 2 niverse CONT'D U 2006INREVIEW A new image from the Galaxy Evolution Explorer completed MARCH a multi-wavelength, neon-col- Cassini found what may be evidence ored portrait of the enormous of liquid water reservoirs that erupt in Cartwheel galaxy after a smaller Yellowstone-like geysers on Saturn’s galaxy plunged through it, trigger- moon Enceladus. -
CONSTELLATION an Official Publication of the Bucks-Mont Astronomical Association, Inc
CONSTELLATION An Official Publication of the Bucks-Mont Astronomical Association, Inc. April/May/June Chris Sommers and VOLUME 23, Issue No. 2 2008 Scott Petersen, Editors © BMAA, Inc. 2008 BMAA News BMAA has had a busy spring, despite almost all of our StarWatches being clouded out. In April we attended an open house at Montgomery County Community College’s Observatory, and Dwight Dulsky and Lou Vittorio made presentations at Upper Moreland Middle School. In May we had our Astronomy Day exhibit set up in Peddler’s Village in New Hope and Dwight Dulsky led the effort at the Bucks County Science Teachers Association’s semi- annual meeting in Doylestown. We have a lot to look forward to this summer, including the summer triangle, summer globular clusters (see Orum Stringer’s List in this Issue) including M56 as described by Alan Pasicznyk, jovial Jupiter and its parade of double shadow transits, and multiple occultations of Antares by the Moon. Happy observing BMAAers!!! Summer Planetary Jewel: Jovial Jupiter Courtesy of Steve Olson BMAA Gophers Position Name President Dwight Dulsky Vice President Bernie Kosher Treasurer Ed Radomski Secretary Herb Borteck Star Watch Coordinator George Reagan Constellation Editors Chris Sommers and Scott Petersen Webmaster Jim Moyer For More Information About BMAA Go to www.bma2.org. 1 ****** Alan's Collection of Excellent Deep Sky Objects Through a 4.5 Inch Newtonian. Raisins in a Pie", M56 ¾ Alan Pasicznyk When I finally located the dim glow of M56 for the first time on July 15, 1991, I was expecting to find nothing more than "just another globular cluster" to log into my list of Messier objects. -
FY 2002 Performance and Accountability Report FY 2002 Was the Second Year of Continuous, Permanent Human Habitation of the International Space Station
National Aeronautics and Space Administration Fiscal Year 2002 Performance and Accountability Report Contents NASAVision and Mission Part I: Management’s Discussion and Analysis Transmittal Letter 6Message From the Administrator 8Reliability and Completeness of Financial and Performance Data 9Federal Managers’ Financial Integrity Act Statement of Assurance Overview 13Mission 13Organizational Structure 15Highlights of Performance Goals and Results 53Actions Planned to Achieve Key Unmet Goals 53Looking Forward 55Analysis of Financial Statements 55Systems, Controls, and Legal Compliance 56Integrity Act Material Weaknesses and Non-Conformances 58Additional Key Management Information 58The President’s Management Agenda 71Management Challenges and High-Risk Areas Part II: Performance 84Summary of Annual Performance by Strategic Goals Performance Discussion 87Space Science 99Earth Science 109Biological and Physical Research 117Human Exploration and Development of Space 123Aerospace Technology Supporting Data 133Space Science 145Earth Science 173Biological and Physical Research 185Human Exploration and Development of Space 193Aerospace Technology 209Manage Strategically Crosscutting Process 219Provide Aerospace Products and Capabilities Crosscutting Process 223Generate Knowledge Crosscutting Process 225Communicate Knowledge Crosscutting Process Part III: Financial 233Letter From the Chief Financial Officer Financial Statements and Related Auditor’s Reports 236Financial Overview 238Financial Statements 267Auditor’s Reports NASA Office of Inspector -
Appendix I Lunar and Martian Nomenclature
APPENDIX I LUNAR AND MARTIAN NOMENCLATURE LUNAR AND MARTIAN NOMENCLATURE A large number of names of craters and other features on the Moon and Mars, were accepted by the IAU General Assemblies X (Moscow, 1958), XI (Berkeley, 1961), XII (Hamburg, 1964), XIV (Brighton, 1970), and XV (Sydney, 1973). The names were suggested by the appropriate IAU Commissions (16 and 17). In particular the Lunar names accepted at the XIVth and XVth General Assemblies were recommended by the 'Working Group on Lunar Nomenclature' under the Chairmanship of Dr D. H. Menzel. The Martian names were suggested by the 'Working Group on Martian Nomenclature' under the Chairmanship of Dr G. de Vaucouleurs. At the XVth General Assembly a new 'Working Group on Planetary System Nomenclature' was formed (Chairman: Dr P. M. Millman) comprising various Task Groups, one for each particular subject. For further references see: [AU Trans. X, 259-263, 1960; XIB, 236-238, 1962; Xlffi, 203-204, 1966; xnffi, 99-105, 1968; XIVB, 63, 129, 139, 1971; Space Sci. Rev. 12, 136-186, 1971. Because at the recent General Assemblies some small changes, or corrections, were made, the complete list of Lunar and Martian Topographic Features is published here. Table 1 Lunar Craters Abbe 58S,174E Balboa 19N,83W Abbot 6N,55E Baldet 54S, 151W Abel 34S,85E Balmer 20S,70E Abul Wafa 2N,ll7E Banachiewicz 5N,80E Adams 32S,69E Banting 26N,16E Aitken 17S,173E Barbier 248, 158E AI-Biruni 18N,93E Barnard 30S,86E Alden 24S, lllE Barringer 29S,151W Aldrin I.4N,22.1E Bartels 24N,90W Alekhin 68S,131W Becquerei -
Mars Earth Return Vehicle (MERV) Propulsion Options
Mars Earth Return Vehicle (MERV) Propulsion Options Steven R. Oleson,1 Melissa L. McGuire,2 Laura Burke,3 James Fincannon,4 Joe Warner,5 Glenn Williams,6 and Thomas Parkey7 NASA Glenn Research Center, Cleveland, Ohio 44135 Tony Colozza,8 Jim Fittje,9 Mike Martini,10 and Tom Packard11 Analex Corporation, Cleveland, Ohio 44135 Joseph Hemminger12 N&R Engineering, Cleveland, Ohio 44135 John Gyekenyesi13 ASRC Engineering, Cleveland, Ohio 44135 The COMPASS Team was tasked with the design of a Mars Sample Return Vehicle. The current Mars sample return mission is a joint National Aeronautics and Space Administration (NASA) and European Space Agency (ESA) mission, with ESA contributing the launch vehicle for the Mars Sample Return Vehicle. The COMPASS Team ran a series of design trades for this Mars sample return vehicle. Four design options were investigated: Chemical Return /solar electric propulsion (SEP) stage outbound, all-SEP, all chemical and chemical with aerobraking. The all-SEP and Chemical with aerobraking were deemed the best choices for comparison. SEP can eliminate both the Earth flyby and the aerobraking maneuver (both considered high risk by the Mars Sample Return Project) required by the chemical propulsion option but also require long low thrust spiral times. However this is offset somewhat by the chemical/aerobrake missions use of an Earth flyby and aerobraking which also take many months. Cost and risk analyses are used to further differentiate the all-SEP and Chemical/Aerobrake options. 1COMPASS Lead, DSB0, 21000 Brookpark Road, and AIAA Senior Member. 2COMPASS Integration Lead, DSB0, 21000 Brookpark Road, non-member. 3Mission Designer, DSB0, 21000 Brookpark Road, and Non-Member. -
Collected Writings
THE DOCUMENTS O F TWENTIETH CENTURY ART General Editor, Jack Flam Founding Editor, Robert Motherwell Other titl es in the series available from University of California Press: Flight Out of Tillie: A Dada Diary by Hugo Ball John Elderfield Art as Art: The Selected Writings of Ad Reinhardt Barbara Rose Memo irs of a Dada Dnnnmer by Richard Huelsenbeck Hans J. Kl ein sc hmidt German Expressionism: Dowments jro111 the End of th e Wilhelmine Empire to th e Rise of National Socialis111 Rose-Carol Washton Long Matisse on Art, Revised Edition Jack Flam Pop Art: A Critical History Steven Henry Madoff Co llected Writings of Robert Mothen/le/1 Stephanie Terenzio Conversations with Cezanne Michael Doran ROBERT SMITHSON: THE COLLECTED WRITINGS EDITED BY JACK FLAM UNIVERSITY OF CALIFORNIA PRESS Berkeley Los Angeles Londo n University of Cali fornia Press Berkeley and Los Angeles, California University of California Press, Ltd. London, England © 1996 by the Estate of Robert Smithson Introduction © 1996 by Jack Flam Library of Congress Cataloging-in-Publication Data Smithson, Robert. Robert Smithson, the collected writings I edited, with an Introduction by Jack Flam. p. em.- (The documents of twentieth century art) Originally published: The writings of Robert Smithson. New York: New York University Press, 1979. Includes bibliographical references and index. ISBN 0-520-20385-2 (pbk.: alk. paper) r. Art. I. Title. II. Series. N7445.2.S62A3 5 1996 700-dc20 95-34773 C IP Printed in the United States of Am erica o8 07 o6 9 8 7 6 T he paper used in this publication meets the minimum requirements of ANSII NISO Z39·48-1992 (R 1997) (Per111anmce of Paper) . -
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center a for Rockets and Satellites
VV D C-A- R 78-03 National Space Science Data Center/ World Data Center A For Rockets and Satellites {NASA-TM-79399) LHNAS TRANSI]_INT PHENOMENA N78-301 _7 CATAI_CG (NASA) 109 p HC AO6/MF A01 CSCl 22_ Unc.las G3 5 29842 NSSDC/WDC-A-R&S 78-03 Lunar Transient Phenomena Catalog Winifred Sawtell Cameron July 1978 National Space Science Data Center (NSSDC)/ World Data Center A for Rockets and Satellites (WDC-A-R&S) National Aeronautics and Space Administration Goddard Space Flight Center Greenbelt) Maryland 20771 CONTENTS Page INTRODUCTION ................................................... 1 SOURCES AND REFERENCES ......................................... 7 APPENDIX REFERENCES ............................................ 9 LUNAR TRANSIENT PHENOMENA .. .................................... 21 iii INTRODUCTION This catalog, which has been in preparation for publishing for many years is being offered as a preliminary one. It was intended to be automated and printed out but this form was going to be delayed for a year or more so the catalog part has been typed instead. Lunar transient phenomena have been observed for almost 1 1/2 millenia, both by the naked eye and telescopic aid. The author has been collecting these reports from the literature and personal communications for the past 17 years. It has resulted in a listing of 1468 reports representing only slight searching of the literature and probably only a fraction of the number of anomalies actually seen. The phenomena are unusual instances of temporary changes seen by observers that they reported in journals, books, and other literature. Therefore, although it seems we may be able to suggest possible aberrations as the causes of some or many of the phenomena it is presumptuous of us to think that these observers, long time students of the moon, were not aware of most of them. -
Cadernos Do CNLF Vol
XI CONGRESSO NACIONAL DE LINGUÍSTICA E FILOLOGIA Círculo Fluminense de Estudos Filológicos e Linguísticos Em Homenagem a Joaquim Mattoso Câmara Jr. UNIVERSIDADE DO ESTADO DO RIO DE JANEIRO (de 27 a 31 de agosto de 2007) Cadernos do CNLF Vol. XI, N° 15 Rio de Janeiro CiFEFiL 2009 A CIDMAR TEODORO PAIS UNIVERSIDADE DO ESTADO DO RIO DE JANEIRO CENTRO DE EDUCAÇÃO E HUMANIDADES FACULDADE DE FORMAÇÃO DE PROFESSORES DEPARTAMENTO DE LETRAS Reitor Ricardo Vieiralves de Castro Vice-Reitora Maria Christina Paixão Maioli Sub-Reitora de Graduação Lená Medeiros de Menezes Sub-Reitora de Pós-Graduação e Pesquisa Monica da Costa Pereira Lavalle Heilbron Sub-Reitora de Extensão e Cultura Regina Lúcia Monteiro Henriques Diretora do Centro de Educação e Humanidades Glauber Almeida de Lemos Diretor da Faculdade de Formação de Professores Maria Tereza Goudard Tavares Vice-Diretor da Faculdade de Formação de Professores Catia Antonia da Silva Chefe do Departamento de Letras Leonardo Pinto Mendes Sub-Chefe do Departamento de Letras Iza Terezinha Gonçalves Quelhas Coordenador de Publicações do Departamento de Letras José Pereira da Silva 2 CADERNOS DO CNLF, VOL. XI, N° 15 Círculo Fluminense de Estudos Filológicos e Linguísticos Círculo Fluminense de Estudos Filológicos e Linguísticos Rua São Francisco Xavier, 512 / 97 – Mangueira – 20943-000 – Rio de Janeiro – RJ [email protected] – (21) 2569-0276 – www.filologia.org.br DIRETOR-PRESIDENTE José Pereira da Silva VICE-DIRETORA Cristina Alves de Brito PRIMEIRA SECRETÁRIA Délia Cambeiro Praça SEGUNDO SECRETÁRIO -
Status of Solar Sail Propulsion: Moving Toward an Interstellar Probe
https://ntrs.nasa.gov/search.jsp?R=20070037462 2019-08-30T01:59:41+00:00Z Status of Solar Sail Propulsion: Moving Toward an Interstellar Probe Les Johnson, Roy M. Young, and Edward E. Montgomery IV NASA George C. Marshall Space Flight Center, Huntsville. AL 35812 Abstract. NASA's In-Space Propulsion Technology Program has developed the first- generation of solar sail propulsion systems sufficient to accomplish inner solar system science and exploration missions. These first-generation solar sails, when operational, will range in size from 40 meters to well over 100 meters in diameter and have an areal density of less than 13 grams-per-square meter. A rigorous, multiyear technology development effort culminated last year in the testing of two different 20-meter solar sail systems under thermal vacuum conditions. This effort provided a number of significant insights into the optimal design and expected performance of solar sails as well as an understanding of the methods and costs of building and using them. In a separate effort, solar sail orbital analysis tools for mission design were developed and tested. Laboratory simulations of the effects of long-term space radiation exposure were also conducted on two candidate solar sail materials. Detailed radia- tion and charging environments were defined for mission trajectories outside the protection of the earth's magnetosphere, in the solar wind environment. These were used in other analytical tools to prove the adequacy of sail design features for accommodating the harsh space environment. Preceding, and in conjunction with these technology efforts, NASA sponsored several mission application studies for solar sails, including one that would use an evolved sail capa- bility to support humanity's first mission into nearby interstellar space.